SH007-08
Inferring Plasma Flows in the Solar Photosphere & Chromosphere using Deep Learning and Surface Observations

Monday, 7 December 2020: 20:58
Virtual
Benoit Tremblay, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States; National Solar Observatory, Tucson, AZ, United States, Kevin Reardon, National Solar Observatory, Boulder, CO, United States, Raphael Attié, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Andrés Asensio Ramos, Instituto de Astrofísica de Canarias, Tenerife, Spain, Maria Kazachenko, University of California Berkeley, Berkeley, CA, United States; University of Colorado at Boulder, LASP, Boulder, CO, United States and Dennis Tilipman, University of Colorado at Boulder, Astrophysical & Planetary Sciences, Boulder, CO, United States
Abstract:
Direct measurements of plasma motions are limited to the line-of-sight component at the Sun's surface. Multiple tracking and inversion methods were developed to infer the transverse motions from observational data. Optical flows do not directly track actual transverse plasma motions, but our most recent results show that unsupervised flow tracking performed on simulation data of the solar surface with the Ball-tracking method accurately reconstructs the true transverse plasma velocity over certain spatial and temporal scales. Recently, the fully convolutional DeepVel & DeepVelU neural networks were trained in conjunction with detailed magnetohydrodynamics (MHD) simulations of the Quiet Sun and sunspots to recover the instantaneous depth/height-dependent transverse velocity vector from a combination of intensitygrams, magnetograms and/or Dopplergrams of the solar surface. Through this supervised learning approach, the neural network attempts to emulate the synthetic flows, and by extension the physics, from the numerical simulation it was presented during its training, i.e. its outputs are model-dependent and may be subjected to biases. Although simulations have become increasingly realistic, the validity of flows inferred by DeepVel or DeepVelU is subject to debate when using real observational data as input. As a test, we use white light images of the Quiet Sun photosphere (optical depth τ=1) produced by the Interferometric BIdimensional Spectropolarimeter (IBIS) installed at the Dunn Solar Telescope to infer plasma motions at optical depth τ=0.1 (i.e., near the transition between the photosphere and the chromosphere) using DeepVelU. We then compare the results to the optical flows determined from a time series of observational data formed near τ=0.1, which may not be subjected to the biases present in DeepVelU. Finally, we discuss work in progress to infer photospheric and chromospheric (optical) flows through unsupervised learning, i.e. learning strictly from observational data and thus without simulations.